Publications (18)
Quantitative spectral analysis of early B-type supergiants in the Sculptor galaxy NGC 300
Miguel Alejandro Urbaneja, Artemio Herrero, Fabio Bresolin +3
Nitrogen line spectroscopy of O-stars -- I. Nitrogen III emission line formation revisited
Jorge G. Rivero Gonzalez, Joachim Puls, Francisco Najarro
The nature and consequences of clumping in hot, massive star winds
Jon O. Sundqvist, Stanley P. Owocki, Joachim Puls
Modeling the early evolution of massive OB stars with an experimental wind routine
Zsolt Keszthelyi, Joachim Puls, Gregg Wade
A proper description of clumping in hot star winds: the key to obtaining reliable mass-loss rates?
Jon O. Sundqvist, Joachim Puls, Achim Feldmeier +1
The Physical Properties and Effective Temperature Scale of O-type Stars as a Function of Metallicity. II. Analysis of 20 More Magellanic Cloud Stars, and Results from the Complete Sample
Philip Massey, Joachim Puls, A. W. A. Pauldrach +3
The Physical Properties and Effective Temperature Scale of O-type Stars as a Function of Metallicity. I. A Sample of 20 Stars in the Magellanic Clouds
Philip Massey, Fabio Bresolin, Rolf P. Kudritzki +2
The Of?p stars of the Magellanic Clouds: Are they strongly magnetic?
Melissa Munoz, Gregg Wade, Yaël Nazé +2
IAU Commission 36 (Theory of Stellar Atmospheres): Hexennial Report 2009-2015
Joachim Puls, Martin Asplund
Very Massive Stars (VMS) in the Local Universe
Jorick S. Vink, Alexander Heger, Mark R. Krumholz +25
The Physical Properties and Effective Temperature Scale of O-type Stars as a Function of Metallicity. III. More Results from the Magellanic Clouds
Philip Massey, Amanda M. Zangari, Nidia I. Morrell +4
Spectroscopic and physical parameters of Galactic O-type stars. III. Mass discrepancy and rotational mixing
Nevena Markova, Joachim Puls, Norbert Langer
A Bake-Off Between CMFGEN and FASTWIND: Modeling the Physical Properties of SMC and LMC O-type Stars
Philip Massey, Kathryn F. Neugent, D. John Hillier +1
OB-stars as extreme condition test beds
Joachim Puls, Jon O. Sundqvist, Jorge G. Rivero González
The influence of clumping on predicted O star wind parameters
Jiri Krticka, Joachim Puls, Jiri Kubat
Towards a unified view of inhomogeneous stellar winds in isolated supergiant stars and supergiant high mass X-ray binaries
Silvia MartÃnez-Núñez, Peter Kretschmar, Enrico Bozzo +13
STIS UV spectroscopy of early B supergiants in M31
Fabio Bresolin, Rolf-Peter Kudritzki, Daniel J. Lennon +4
Stellar Winds in Massive X-ray Binaries
Peter Kretschmar, Silvia MartÃnez-Núñez, Enrico Bozzo +15